| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.47 | 193.61 | 16.06 | 102.68 | 19.80 | 103.73 | -7.57 | 20.54 | 0.3559 | -809.0 | -411.6 | |
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back to the solar disc SDO HMI 2011-12-05 03:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.56 | 23.81 | 105.95 | -5.35 | 12.12 | 0.4081 | -724.0 | -611.2 | |
| 0.00 | 2.47 | 0.00 | 1.35 | 24.75 | 104.73 | -6.57 | 14.14 | 0.4269 | -746.0 | -673.0 | |
| 30.47 | 168.55 | 16.06 | 88.84 | 19.06 | 104.02 | -7.28 | 20.54 | 0.3431 | -1297.0 | -427.6 | |
| 0.00 | 1.11 | 0.00 | 0.60 | 23.13 | 103.49 | -7.81 | 17.93 | 0.4079 | -758.0 | -649.8 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 19.75 | 103.48 | -7.82 | 21.14 | 0.3567 | -427.0 | -334.1 | |
| 0.00 | 4.01 | 0.00 | 2.23 | 25.95 | 102.81 | -8.49 | 17.11 | 0.4532 | -836.0 | -636.4 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 25.56 | 102.31 | -8.99 | 18.35 | 0.4498 | -206.0 | -271.7 | |
| 0.00 | 1.19 | 0.00 | 0.67 | 26.25 | 102.02 | -9.28 | 18.35 | 0.4613 | -820.0 | -713.6 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 19.90 | 102.36 | -8.94 | 23.64 | 0.3660 | 807.0 | 523.6 | |
| 0.00 | 3.41 | 0.00 | 1.91 | 26.22 | 101.69 | -9.61 | 18.98 | 0.4624 | -874.0 | -723.5 | |
| 0.00 | 1.28 | 0.00 | 0.74 | 30.02 | 100.82 | -10.48 | 17.68 | 0.5209 | -622.0 | -431.7 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 29.92 | 100.45 | -10.85 | 18.32 | 0.5212 | -626.0 | -507.4 | |
| 0.00 | 1.62 | 0.00 | 0.95 | 30.43 | 99.31 | -12.00 | 19.70 | 0.5338 | -679.0 | -575.7 | |
| 0.00 | 1.62 | 0.00 | 0.86 | 18.40 | 99.18 | -12.12 | 32.81 | 0.3693 | 820.0 | 693.4 | |
| 0.00 | 1.96 | 0.00 | 1.04 | 18.21 | 99.16 | -12.14 | 33.14 | 0.3670 | 855.0 | 710.7 | |
| 0.00 | 0.94 | 0.00 | 0.50 | 18.37 | 98.77 | -12.53 | 33.72 | 0.3726 | 539.0 | 431.1 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |